A dataset provided by the European Space Agency

Name: The X-ray timing behaviour of the radio-quiet PSR J1809-2332 in the Taz nebula
Published: 2017-05-11T22:00:00Z

Proposal ID	076388
Title	The X-ray timing behaviour of the radio-quiet PSR J1809-2332 in the Taz nebula
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763880101
DOI	https://doi.org/10.5270/esa-w20rkrv
Principal Investigator, PI	Dr Massimiliano Razzano
Abstract	The study of radio-quiet gamma-ray pulsars discovered by the Fermi Large AreaTelescope is key for pulsar magnetosphere and Galactic neutron star populationmodels. We propose a deep xmm observation of PSR J1809-2332, the radio-quietpulsar in the Taz nebula. Its timing parameters and gamma-ray properties makeit a transition object between the young, Vela-like, and the middle-aged,Geminga-like, pulsars. Thus, studying its X and gamma-ray emission is crucial toprobe the radio quietness/loudness in pulsars of different ages. We will use XMMto search for X-ray pulsations from PSR J1809-2332, detail its timing andspectral properties, and resolve its emission from that of its nebula by usingalso archival Chandra data.
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-04-06T05:07:57Z/2016-04-07T17:27:57Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2017-05-11T22:00:00Z
Last Update	2025-01-27
Keywords	"transition object", "archival chandra data", "gamma ray properties", "pulsar magnetosphere", "middle aged", "radio quietness", "xray pulsations", "psr j1809 2332", "radio quiet pulsar", "spectral properties", "gamma ray emission", "deep xmm", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Massimiliano Razzano, 2017, 'The X-ray timing behaviour of the radio-quiet PSR J1809-2332 in the Taz nebula', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w20rkrv